Datum verslag: 2025 Aug 27 1231 UTC
M-class flares expected (probability >=50%)
Active conditions expected (A>=20 or K=4)
Proton event expected (10 pfu at >10 MeV)
| 10cm flux | Ap | |
|---|---|---|
| 27 Aug 2025 | 202 | 007 |
| 28 Aug 2025 | 202 | 007 |
| 29 Aug 2025 | 202 | 007 |
Solar flaring activity was moderate over the past 24 hours, with 1 M-class flare identified. This was an M1.0 flare (SIDC Flare 5239) peaking on August 26 at 14:07 UTC, which was produced by SIDC Sunspot Group 592 (NOAA Active Regions 4202). A total of 14 numbered sunspot groups were identified on the disk over the past 24 hours. Solar flaring activity is expected to be moderate over the next 24 hours, with M-class flares likely.
No Earth-directed Coronal Mass Ejections (CMEs) have been observed in the last 24 hours.
SIDC Coronal Hole 126 (northern mid-latitude coronal hole with negative polarity) is located in the western hemisphere, its associated high speed stream may still reach the Earth today.
The Earth is inside slow solar wind with speeds around 350 km/s and interplanetary magnetic fields of about 7 nT (directed towards the Sun, negative polarity). The high speed stream from SIDC Coronal Hole 126 has not arrived to the Earth, it may still do so today (with minor influence expected).
Geomagnetic conditions have been quiet (Kp and B_Bel between 0 and 2). Quiet to unsettled periods are expected for the next 24 hours.
The greater than 10 MeV proton flux passed above the 10 pfu threshold on 26 August, and is currently at 12 pfu. The proton levels started to slowly increase on 22 August (as the result of a backsided CME on 21 August) and have gradually approached the threshold. Since 25 August the levels were very close to the 10 pfu mark. The flux will remain elevated in the next 24 hours, but no strong additional increases are expected.
The greater than 2 MeV electron flux as measured by GOES 18 and 19 remained below the 1000 pfu alert threshold, similar conditions expected for the next 24 hours. The 24 h electron fluence was at normal levels and is expected to remain so.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 199, gebaseerd op 12 stations.
| Wolfgetal Catania | 172 |
| 10cm zonneflux | 202 |
| AK Chambon La Forêt | 011 |
| AK Wingst | 008 |
| Geschatte Ap | 009 |
| Geschat internationaal zonnevlekkengetal | 187 - Gebaseerd op 26 stations |
| Dag | Start | Max | Einde | Locatie | Sterkte | OP | 10cm | Catania/NOAA | Soorten radio-uitbarstingen |
|---|---|---|---|---|---|---|---|---|---|
| 26 | 1339 | 1407 | 1432 | ---- | M1.0 | --/4202 | III/1VI/1 |
Aangeboden door het Solar Influences Data Analysis Center© - SIDC - Verwerkt door SpaceWeatherLive
Alle tijden in UTC
<< Keer terug naar de dagelijkse overview pagina
Veel mensen komen naar Poollicht.be om de zonneactiviteit te volgen of om het poollicht te zien, maar met meer bezoekers komen er hogere kosten bij om de servers online te houden. Als je Poollicht.be leuk vindt en het project wilt steunen, kun je kiezen voor een abonnement op een advertentievrije website of een donatie overwegen. Met jouw hulp kunnen we Poollicht. be online houden!
| Laatste X-klasse uitbarsting | 01/02/2026 | X1.0 |
| Laatste M-klasse uitbarsting | 01/02/2026 | M1.5 |
| Laatste geomagnetische storm | 28/01/2026 | Kp5+ (G1) |
| Zonnevlekkenloze dagen | |
|---|---|
| Laatste zonnevlekkenloze dag | 08/06/2022 |
| Maandelijks gemiddeld zonnevlekkengetal | |
|---|---|
| december 2025 | 124 +32.2 |
| Afgelopen 30 dagen | 119.2 +2.7 |